Radial velocity follow-up for confirmation and characterization of transiting exoplanets
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Radial Velocity follow-up is essential to establish or exclude the planetary nature of a transiting companion as well as to accurately determine its mass. Here we present some elements of an efficient Doppler follow-up strategy, based on high-resolution spectroscopy, devoted to the characterization of transiting candidates. Some aspects and results of the radial velocity follow-up of the CoRoT space mission are presented in order to illustrate the strategy used to deal with the zoo of transiting candidates.
10 pages, proceedings IAU symposium 253, Boston, May 2008
10 pages, proceedings IAU symposium 253, Boston, May 2008